Linear Polarisation Properties of Pulsars at 35 & 327 MHz

Astronomy and Astrophysics – Astrophysics

Scientific paper

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2 pages, 4 figures, To appear in the Proceedings of IAU Colloquium 177 : "Pulsar Astronomy - 2000 & Beyond", Ed. Kramer, Wex,

Scientific paper

We report preliminary results of our study of linear polarization in the
pulsar emission at 35 & 327 MHz. We have exploited for this purpose the
spectral modulation resulting from the differential Faraday rotation across the
observed band. We discuss the results on a few bright pulsars by comparing them
with the existing measurements at higher radio frequencies.

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